Download Angular momentum

Angular momentum
Quantum mechanics
1)) Orbital angular momentum
)
Consider a particle described by the Cartesian coordinates (x, y, z) ≡ r and their
conjugate momenta (px , py , pz ) ≡ p. The classical definition of the orbital angular
momentum of such a particle about the origin is L = r × p, giving
Lx = y p z − z p y ,
(1)
Ly = z p x − x p z ,
(2)
Lz = x p y − y p x .
(3)
Let us assume that the operators (Lx , Ly , Lz ) ≡ L which represent the components of orbital angular momentum in quantum mechanics can be defined in an
analogous manner to the corresponding components of classical angular momentum. In other words, we are going to assume that the above equations specify
the angular momentum operators in terms of the position and linear momentum
operators. Note that Lx , Ly , and Lz are Hermitian, so they represent things which
can, in principle, be measured. Note, also, that there is no ambiguity regarding the order in which operators appear in products on the right-hand sides
Eqs. (1)–(3), since all of the products consist of operators which commute.
The fundamental commutation relations satisfied by the position and linear
momentum operators are
[xi , xj ] = 0,
(4)
[pi , pj ] = 0,
(5)
[xi , pj ] = i h̄ δij ,
(6)
where i and j stand for either x, y, or z. Consider the commutator of the operators
Lx and Lz :
[Lx , Ly ] = [(y pz − z py ), (z px − x pz )] = y [pz , z] px + x py [z, pz ]
= i h̄ (−y px + x py ) = i h̄ Lz .
Quantum mechanics
Orbital angular momentum
The cyclic permutations of the above result yield the fundamental commutation
relations satisfied by the components of an angular momentum:
[Lx , Ly ] = i h̄ Lz ,
(8)
[Ly , Lz ] = i h̄ Lx ,
(9)
[Lz , Lx ] = i h̄ Ly .
(10)
These can be summed up more succinctly by writing
L × L = i h̄ L.
(11)
The three commutation relations (8 )–(10 ) are the foundation for the whole
theory of angular momentum in quantum mechanics. Whenever we encounter
three operators having these commutation relations, we know that the dynamical
variables which they represent have identical properties to those of the components of an angular momentum (which we are about to derive). In fact, we shall
assume that any three operators which satisfy the commutation relations (8 )–
(10 ) represent the components of an angular momentum.
Suppose that there are N particles in the system, with angular momentum
vectors Li (where i runs from 1 to N). Each of these vectors satisfies Eq. (11 ),
so that
Li × Li = i h̄ Li .
(12)
However, we expect the angular momentum operators belonging to different particles to commute, since they represent different degrees of freedom of the system. So, we can write
Li × Lj + Lj × Li = 0,
(13)
PN
for i 6= j. Consider the total angular momentum of the system, L = i=1 Li . It is
clear from Eqs. (12 ) and (13 ) that
L×L =
N
X
i=1
= i h̄
Li ×
N
X
i=1
N
X
Lj =
j=1
Li = i h̄ L.
N
X
i=1
N
1X
Li × L i +
(Li × Lj + Lj × Li )
2 i,j=1
Quantum mechanics
Orbital angular momentum
Consider the magnitude squared of the angular momentum vector, L2 ≡ Lx2 +
L 2 + Lz2 . The commutator of L2 and Lz is written
y
[L2 , Lz ] = [Lx2 , Lz ] + [Ly2 , Lz ] + [Lz2 , Lz ].
(15)
It is easily demonstrated that
[Lx2 , Lz ] = −i h̄ (Lx Ly + Ly Lx ),
(16)
[Ly2 , Lz ] = +i h̄ (Lx Ly + Ly Lx ),
(17)
[Lz2 , Lz ] = 0,
(18)
so
[L2 , Lz ] = 0.
(19)
Since there is nothing special about the z-axis, we conclude that L 2 also commutes
with Lx and Ly . It is clear from Eqs. ( 8 )–(10 ) and (19 ) that the best we can
do in quantum mechanics is to specify the magnitude of an angular momentum
vector along with one of its components (by convention, the z-component).
It is convenient to define the shift operators L+ and L− :
L+ = L x + i L y ,
(20)
L− = L x − i L y .
(21)
[L+ , Lz ] = −h̄ L+ ,
(22)
[L− , Lz ] = +h̄ L− ,
(23)
[L+ , L− ] = 2 h̄ Lz .
(24)
Note that
Note, also, that both shift operators commute with L2 .
Eigenfunctions of orbital angular momentum
Quantum mechanics
Eigenfunctions of orbital angular momentum
In Cartesian coordinates, the three components of orbital angular momentum can
be written
26
!
Lz
!
!
Ly
!
Lx
∂
∂
−z
= −i h̄ y
∂z
∂y
!
∂
∂
−x
= −i h̄ z
∂x
∂z
!
∂
∂
= −i h̄ x
−y
∂y
∂x
using the Schrödinger representation. Transforming to standard spherical polar
coordinates,
x = r sin θ cos ϕ,
(27)
(28)
(29)
y = r sin θ sin ϕ,
z = r cos θ,
Ly
Lz
∂
∂
+ cot θ cos ϕ
= i h̄ sin ϕ
∂θ
∂ϕ
!
Lx
!
we obtain
!
∂
∂
− cot θ sin ϕ
= −i h̄ cos ϕ
∂θ
∂ϕ
∂
.
= −i h̄
∂ϕ
(30)
!
(31)
(32)
(33)
L2 = Lx2 + Ly2 + Lz2
from the above eqs. (30), (31) , (32) and (34), we can obtain:
1 ∂
∂
1 ∂2 
L2 = −h̄2 
sin θ
+
.
sin θ ∂θ
∂θ sin2 θ ∂ϕ2


(34)
Eigenfunctions of orbital angular momentum
Quantum
The eigenvalue problem for L2 takes the form
L2 ψ = λ h̄2 ψ,
(35)
where ψ(r, θ, ϕ is the wave-function, and λ is a number. Let us write
(r, θ, ϕ) = R(r) Y(θ, ϕ).
(36)
1 ∂
∂
1 ∂2 

sin θ
+
Y + λ Y = 0,
sin θ ∂θ
∂θ sin2 θ ∂ϕ2
(37)
Equation (35) reduces to


where use has been made of Eq. (34) As is well-known, square integrable
solutions to this equation only exist when λ takes the values l (l + 1), where l is
an integer. These solutions are known as spherical harmonics, and can be written
Ylm (θ, ϕ) =
v
u
u2 l
u
t
+ 1 (l − m)!
(−1)m e i m ϕ Plm (cos ϕ),
4π (l + m)!
(38)
where m is a positive integer lying in the range 0 ≤ m ≤ l. Here, Plm (ξ) is an
associated Legendre function satisfying the equation
m
m2 m
d
2 dPl
Pl + l (l + 1) Plm = 0.
(1 − ξ )
−
2
dξ
dξ
1−ξ
"
#
We define
Yl−m = (−1)m (Ylm )∗ ,
(40)
(41)
which allows m to take the negative values −l ≤ m < 0. The spherical harmonics
are orthogonal functions, and are properly normalized with respect to integration
over the entire solid angle:
Z π Z 2π
0
(42)
Ylm∗ (θ, ϕ) Ylm0 (θ, ϕ) sin θ dθ dϕ = δll 0 δmm 0 .
0
0
Eigenfunctions of orbital angular momentum
Quantum mechanics
The spherical harmonics also form a complete set for representing general functions of θ and ϕ.
By definition,
L2 Ylm = l (l + 1) h̄2 Ylm ,
(43)
where l is an integer. It follows from Eqs. (32)and (38) that
Lz Ylm = m h̄ Ylm ,
(44)
where m is an integer lying in the range −l ≤ m ≤ l. Thus, the wave-function
(r, θ, ϕ) = R(r) Ylm (θ, φ), where R is a general function, has all of the expected
features of the wave-function of a simultaneous eigenstate of L2 and Lz belonging
to the quantum numbers l and m.